Solar Particle Events Observation Capabilities of PAMELA Experiment

Details Solar Particle Events Observation Capabilities of PAMELA Experiment Solar Particle Events Observation Capabilities of PAMELA Experiment

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....6.3477c&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

Scientific paper

PAMELA is a satellite borne experiment to be launched in low Earth orbit on board of the ResursDK1 Russian satellite in the early of the year 2003. It consists of a permanent magnet core, a Transition Radiation Detector, a Time of flight system and a Silicon Tungsten tracking calorimeter. Its main aim is the investigation of the cosmic radiation: origin and evolution of matter in the galaxy, search for antimatter and dark matter of cosmological significance, understanding of origin and acceleration of relativistic particles in the galaxy. The detector can however be used also to address issues relative to the solar terrestrial environment (ab ove 50 MeV) such as Solar particle events (isotopic composition of H and He, eand e+ spectrum) and composition and temporal dependence of the trapped and albedo particle component. In this work we will describe the observational capabilities of PAMELA in presence of solar particle events.

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